S5 Retrograde Initial Condition Case

The S5 retrograde initial condition case is given by these set of parameters, which will also be the same for the direct case. The $X$ and $Y$ are the Cartesian coordinates, in kiloparsecs, of the disrupting galaxy $S$ at the apex of the parabola while $U$ and $V$ are the velocity components. With $X = 1$, the $X$ position of $S$ should be around $25 \: kpc$. The eccentricity of the condition is $1$, which indicates the path will be parabolic.

Type	Position $X$	Position $Y$	Velocity $U$	Velocity $V$	Eccentricity $\epsilon_s$	Mass ratio $S/M$
S5	1	0	0	> 0	1	1

To calculate and solve the equations for this case wasn't too hard. I only needed to modify the original parabolic function to satisfy the conditions set out.

Initial Condition and Solutions Code:

S5 Initial Conditions and Solutions



In [4]:

    
direct_r1, direct_r2, retro_r1, retro_r2, R1, R2, vR1, vR2 = S5_ode_solutions(t,tsteps,M,S,gamma)



In [1]:

    
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
import seaborn as sns
import timeit
from scipy.integrate import odeint
from IPython.html.widgets import interact, fixed
from moviepy.video.io.bindings import mplfig_to_npimage
import moviepy.editor as mpy









    



:0: FutureWarning: IPython widgets are experimental and may change in the future.
WARNING:py.warnings:/usr/local/lib/python3.4/dist-packages/skimage/filter/__init__.py:6: skimage_deprecation: The `skimage.filter` module has been renamed to `skimage.filters`.  This placeholder module will be removed in v0.13.
  warn(skimage_deprecation('The `skimage.filter` module has been renamed '



In [2]:

    
gamma = 4.4983169634398597e4
tsteps = 1000
t = np.linspace(0,1.5,tsteps)
M = 10
S = 10
whichplot='retro'



In [3]:

    
from derivsfunc import *
from initialconditions import *
from S5_icsandsolutions import *
from S5static import *
from S5retromoviemaker import *;

To confirm that my solution of the conditions indicated in the above table are correct, or close to correct, here are my results. As we can see, the positions and velocities are either spot on or relatively close to the requested value.



In [7]:

    
print("X position: %f kpc" % (R1[192]))
print("Y position: %f kpc" % (R2[192]))
print("U velocity: %f kpc/yr" % (vR1[192]))
print("V velocity: %f kpc/yr" % (vR2[192]))









    



X position: 24.999750 kpc
Y position: 0.158064 kpc
U velocity: -0.848096 kpc/yr
V velocity: 268.275293 kpc/yr

In this case, the effect of galaxy $S$ on the system is similar to that of the original base case, with the only change being the direction of motion of $S$.

S5 Static Plotter



In [4]:

    
S5_plot_static(t,whichplot,tsteps,M,S,gamma)

S5 Retrograde Movie Maker



In [5]:

    
S5retro_animation.ipython_display(fps=60)









    









    Out[5]: